IersTechnicalNote36RelativisticCorrectionForce Properties |
The IersTechnicalNote36RelativisticCorrectionForce type exposes the following members.
Properties| Name | Description | |
|---|---|---|
 | CentralBody |
Gets or sets the CentralBody about which this correction is applied.
|
| CentralBodyAngularMomentumPerUnitMass |
Gets or sets a vector that describes the angular momentum per unit mass of the CentralBody. This vector is used for the
Lense-Thirring correction, and may be safely ignored if this term is not used. Two easy-to-use static helper methods for this vector exist on this class;
RouthsRuleAngularMomentumPerUnitMass(CentralBody) and ScaledAngularVelocityAngularMomentumPerUnitMass(CentralBody, Double).
|
| CentralBodyGravitationalParameter |
Gets or sets the gravitational parameter for the CentralBody.
|
| ForceVector |
Gets the Vector representation of this force.
(Inherited from ForceModel.) |
| IsFrozen |
Gets a value indicating whether this object is frozen. A frozen object cannot be modified and an
ObjectFrozenException will be thrown if an attempt is made to do so.
(Inherited from DefinitionalObject.) |
| Kind |
Gets an enumeration indicating the nature of this force and whether it implicitly
includes mass.
(Inherited from ForceModel.) |
| Role |
Gets the role that this force plays in a combined resultant force. In particular, it indicates
whether this force is dominant and easy to compute or whether it is a small perturbation that
is expensive to compute.
(Inherited from ForceModel.) |
| SolarCentralBody |
Gets or sets the CentralBody that represents the sun of the solar system where this force is used.
|
| SolarGravitationalParameter |
Gets or sets the gravitational parameter for the Sun.
|
| TargetPoint |
Gets or sets the point at which the IersTechnicalNote36RelativisticCorrectionForce is applied.
|
| UseDeSitterCorrection |
Gets or sets a value indicating whether the de Sitter correction is to be used. This defaults to
.
|
| UseLenseThirringCorrection |
Gets or sets a value indicating whether the Lense-Thirring correction is to be used. This defaults to
.
|
See Also